504 research outputs found

    Surface and vortex structures in noncentrosymmetric superconductors under applied magnetic fields

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    We investigate how the macroscopic spatial structure of broken inversion symmetry manifests in noncentrosymmetric superconductors, by the microscopic broken inversion symmetry of the crystal structure. Based on the time-dependent Ginzburg-Landau theory including the Pauli paramagnetic effect and the Rashba interaction, we demonstrate that the centrosymmetric structures of the internal field and the screening current are broken macroscopically. The flow structure of paramagnetic supercurrent spontaneously induce the flux flow without applying external currents.Comment: 5 pages, 8 figures. accepted in Phys. Rev.

    Nuclear Magnetic Relaxation Rate in a Noncentrosymmetric Superconductor

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    For a noncentrosymmetric superconductor such as CePt3Si, we consider a Cooper pairing model with a two-component order parameter composed of spin-singlet and spin-triplet pairing components. We demonstrate that such a model on a qualitative level accounts for experimentally observed features of the temperature dependence of the nuclear spin-lattice relaxation rate 1/T1, namely a peak just below Tc and a line-node gap behavior at low temperatures.Comment: 4 page

    Magnetic Properties of a Superconductor with no Inversion Symmetry

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    We study the magnetic properties of a superconductor in a crystal without z→−zz \to -z symmetry, in particular how the lack of this symmetry exhibits itself. We show that, though the penetration depth itself shows no such effect, for suitable orientation of magnetic field, there is a magnetic field discontinuity at the interface which shows this absence of symmetry. The magnetic field profile of a vortex in the x−yx-y plane is shown to be identical to that of an ordinary anisotropic superconductor except for a shift in the −z-z direction by κ~λx{\tilde \kappa} \lambda_x (see errata). For a vortex along zz, there is an induced magnetization along the radial direction.Comment: J. Low Temp. Physics, 140, 67 (2005); with Errat

    Spin susceptibility in superconductors without inversion symmetry

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    In materials without spatial inversion symmetry the spin degeneracy of the conduction electrons can be lifted by an antisymmetric spin-orbit coupling. We discuss the influence of this spin-orbit coupling on the spin susceptibility of such superconductors, with a particular emphasis on the recently discovered heavy Fermion superconductor CePt3Si. We find that, for this compound (with tetragonal crystal symmetry,) irrespective of the pairing symmetry, the stable superconducting phases would give a very weak change of the spin susceptibility for fields along the c-axis and an intermediate reduction for fields in the basal plane. We also comment on the consequences for the paramagnetic limiting in this material.Comment: 10 pages, 3 figure

    Spectrophotometric properties of dwarf planet Ceres from the VIR spectrometer on board the Dawn mission

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    We study the spectrophotometric properties of dwarf planet Ceres in the VIS-IR spectral range by means of hyper-spectral images acquired by the VIR imaging spectrometer on board the NASA Dawn mission. Disk-resolved observations with a phase angle within the 7∘<α<132∘7^{\circ}<\alpha<132^{\circ} interval were used to characterize Ceres' phase curve in the 0.465-4.05 μ\mum spectral range. Hapke's model was applied to perform the photometric correction of the dataset, allowing us to produce albedo and color maps of the surface. The VV-band magnitude phase function of Ceres was fitted with both the classical linear model and H-G formalism. The single-scattering albedo and the asymmetry parameter at 0.55μ\mum are w=0.14±0.02w=0.14\pm0.02 and ξ=−0.11±0.08\xi=-0.11\pm0.08, respectively (two-lobe Henyey-Greenstein phase function); the modeled geometric albedo is 0.094±0.0070.094\pm0.007; the roughness parameter is θˉ=29∘±6∘\bar{\theta}=29^{\circ}\pm6^{\circ}. Albedo maps indicate small variability on a global scale with an average reflectance of 0.034±0.0030.034 \pm 0.003. Isolated areas such as the Occator bright spots, Haulani, and Oxo show an albedo much higher than average. We measure a significant spectral phase reddening, and the average spectral slope of Ceres' surface after photometric correction is 1.1%kA˚−11.1\%k\AA^{-1} and 0.85%kA˚−10.85\%k\AA^{-1} at VIS and IR wavelengths, respectively. Broadband color indices are V−R=0.38±0.01V-R=0.38\pm0.01 and R−I=0.33±0.02R-I=0.33\pm0.02. H-G modeling of the VV-band magnitude phase curve for α<30∘\alpha<30^{\circ} gives H=3.14±0.04H=3.14\pm0.04 and G=0.10±0.04G=0.10\pm0.04, while the classical linear model provides V(1,1,0∘)=3.48±0.03V(1,1,0^{\circ})=3.48\pm0.03 and β=0.036±0.002\beta=0.036\pm0.002. The comparison with spectrophotometric properties of other minor bodies indicates that Ceres has a less back-scattering phase function and a slightly higher albedo than comets and C-type objects. However, the latter represents the closest match in the usual asteroid taxonomy.Comment: 14 pages, 20 figures, published online on Astronomy and Astrophysics on 13 February 2017. Revised to reflect minor changes in text and figures made in proofs, updated value of V-R and R-

    Anomalous Spin Response in Non-centrosymmetric Compounds

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    We examine static spin susceptibilities χαβ(q)\chi_{\alpha\beta}({\bf q}) of spin components SαS_{\alpha} and SβS_{\beta} in the non-centrosymmetric tetragonal system. These show anomalous momentum dependences like χxx(q)−χyy(q)∼qx2−qy2\chi_{xx}({\bf q})-\chi_{yy}({\bf q})\sim q_x^2-q_y^2 and χxy(q)+χyx(q)∼qxqy\chi_{xy}({\bf q})+\chi_{yx}({\bf q})\sim q_x q_y, which vanish in centrosymmetric systems. The magnitudes of the anomalous spin susceptibilities are enhanced by the on-site Coulomb interaction, especially, around an ordering wave vector. The significant and anomalous momentum dependences of these susceptibilities are explained by a group theoretical analysis. As the direct probe of the anomalous spin susceptibility, we propose a polarized neutron scattering experiment.Comment: 4 pages, 1 table, 4 figure

    Novel Pressure Phase Diagram of Heavy Fermion Superconductor CePt3_{3}Si Investigated by ac Calorimetry

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    The pressure dependences of the antiferromagnetic and superconducting transition temperatures have been investigated by ac heat capacity measurement under high pressures for the heavy-fermion superconductor CePt3_3Si without inversion symmetry in the tetragonal structure. The N\'{e}el temperature TNT_{\rm N} = 2.2 K decreases with increasing pressure and becomes zero at the critical pressure PAFP_{\rm AF} ≃\simeq 0.6 GPa. On the other hand, the superconducting phase exists in a wider pressure region from ambient pressure to about 1.5 GPa. The pressure phase diagram of CePt3_3Si is thus very unique and has never been reported before for other heavy fermion superconductors.Comment: 4 pages and 3 figures. This paper will be published in the July issue of J. Phys. Soc. Jp

    Reduction of Pauli paramagnetic pair-breaking effect in antiferromagnetic superconductors

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    Antiferromagnetic superconductors in a magnetic field are studied. We examine a mechanism which significantly reduces the Pauli paramagnetic pair-breaking effect. The mechanism is realized even in the presence of the orbital pair-breaking effect. We illustrate it using a three-dimensional model with an intercalated magnetic subsystem. The upper critical field is calculated for various parameters. It is shown that the upper critical field can reach several times the pure Pauli paramagnetic limit. The possible relevance to the large upper critical field observed in the heavy fermion antiferromagnetic superconductor CePt_3Si discovered recently is briefly discussed. We try to understand the large upper critical field in the compound CePt_3Si and field-induced superconductivity in the compound CePb_3 within a unified framework.Comment: 5 pages, 2 figures, revtex4, minor correction

    Absence of Aquaporin-4 in Skeletal Muscle Alters Proteins Involved in Bioenergetic Pathways and Calcium Handling

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    Aquaporin-4 (AQP4) is a water channel expressed at the sarcolemma of fast-twitch skeletal muscle fibers, whose expression is altered in several forms of muscular dystrophies. However, little is known concerning the physiological role of AQP4 in skeletal muscle and its functional and structural interaction with skeletal muscle proteome. Using AQP4-null mice, we analyzed the effect of the absence of AQP4 on the morphology and protein composition of sarcolemma as well as on the whole skeletal muscle proteome. Immunofluorescence analysis showed that the absence of AQP4 did not perturb the expression and cellular localization of the dystrophin-glycoprotein complex proteins, aside from those belonging to the extracellular matrix, and no alteration was found in sarcolemma integrity by dye extravasation assay. With the use of a 2DE-approach (BN/SDS-PAGE), protein maps revealed that in quadriceps, out of 300 Coomassie-blue detected and matched spots, 19 proteins exhibited changed expression in AQP4−/− compared to WT mice. In particular, comparison of the protein profiles revealed 12 up- and 7 down-regulated protein spots in AQP4−/− muscle. Protein identification by MS revealed that the perturbed expression pattern belongs to proteins involved in energy metabolism (i.e. GAPDH, creatine kinase), as well as in Ca2+ handling (i.e. parvalbumin, SERCA1). Western blot analysis, performed on some significantly changed proteins, validated the 2D results. Together these findings suggest AQP4 as a novel determinant in the regulation of skeletal muscle metabolism and better define the role of this water channel in skeletal muscle physiology

    Emergent Nodal Excitations due to the Coexistence of Superconductivity and Antiferromagnetism: Cases with and without Inversion Symmetry

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    We argue the emergence of nodal excitations due to the coupling with static antiferromagnetic order in fully-gapped superconducting states in both cases with and without inversion symmetry. This line node structure is not accompanied with the sign change of the superconducting gap, in contrast to usual unconventional Cooper pairs with higher angular momenta. In the case without inversion symmetry, the stability of the nodal excitations crucially depends on the direction of the antiferromagnetic staggered magnetic moment. A possible realization of this phenomenon in CePt3_3Si is discussed.Comment: 4 pages, 7 figure
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